Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Rui Curado da Silva"'
Autor:
Andrzej A. Zdziarski, Andrei M. Bykov, Irfan Kuvvetli, G. Kanbach, Dieter H. Hartmann, A. Argan, Silvia Zane, Andrea Bulgarelli, Andreas Zoglauer, Julie McEnery, Kazuhiro Nakazawa, Peter von Ballmoos, Søren Brandt, Alessandro De Angelis, M. N. Mazziotta, Vincent Tatischeff, Marco Tavani, M. Hernanz, Elisa Costantini, Uwe Oberlack, Javier Rico, Lorraine Hanlon, Philippe Laurent, Isabelle Grenier, Rui Curado da Silva, R. Walter, A. Morselli, Mark Pearce, Xin Wu
Publikováno v:
Exper.Astron.
Exper.Astron., 2021, 51 (3), pp.1225-1254. ⟨10.1007/s10686-021-09706-y⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
De Angelis, A, Tatischeff, V, Argan, A, Brandt, S, Bulgarelli, A, Bykov, A, Costantini, E, Silva, R C D, Grenier, I A, Hanlon, L, Hartmann, D, Hernanz, M, Kanbach, G, Kuvvetli, I, Laurent, P, Mazziotta, M N, McEnery, J, Morselli, A, Nakazawa, K, Oberlack, U, Pearce, M, Rico, J, Tavani, M, Ballmoos, P V, Walter, R, Wu, X, Zane, S, Zdziarski, A & Zoglauer, A 2021, ' Gamma-ray astrophysics in the MeV range : The ASTROGAM concept and beyond ', Experimental Astronomy, vol. 51, pp. 1225–1254 . https://doi.org/10.1007/s10686-021-09706-y
Exper.Astron., 2021, 51 (3), pp.1225-1254. ⟨10.1007/s10686-021-09706-y⟩
Digital.CSIC. Repositorio Institucional del CSIC
instname
De Angelis, A, Tatischeff, V, Argan, A, Brandt, S, Bulgarelli, A, Bykov, A, Costantini, E, Silva, R C D, Grenier, I A, Hanlon, L, Hartmann, D, Hernanz, M, Kanbach, G, Kuvvetli, I, Laurent, P, Mazziotta, M N, McEnery, J, Morselli, A, Nakazawa, K, Oberlack, U, Pearce, M, Rico, J, Tavani, M, Ballmoos, P V, Walter, R, Wu, X, Zane, S, Zdziarski, A & Zoglauer, A 2021, ' Gamma-ray astrophysics in the MeV range : The ASTROGAM concept and beyond ', Experimental Astronomy, vol. 51, pp. 1225–1254 . https://doi.org/10.1007/s10686-021-09706-y
Angelis, A. de, et al.
The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics. In particular, (1) it is the missing ingredient for understanding extreme processes in the multi-messenger era; (2)
The energy range between about 100 keV and 1 GeV is of interest for a vast class of astrophysical topics. In particular, (1) it is the missing ingredient for understanding extreme processes in the multi-messenger era; (2)
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e8f812057d32d59399cf673e5ef95be2
https://hal.archives-ouvertes.fr/hal-03150563
https://hal.archives-ouvertes.fr/hal-03150563
Autor:
Barbara Patricelli, V. Bonvicini, Riccardo Rando, Sandro Mereghetti, Andrea Vacchi, Kazuhiro Nakazawa, Claudio Labanti, Jordi Isern, M. Hayashida, Josep M. Paredes, J. Eric Grove, C. Hamadache, Andreas Zoglauer, Olivier Limousin, Julie McEnery, Andrei M. Bykov, G. Ambrosi, D. de Martino, Francesco Longo, Irfan Kuvvetli, Alexander Moiseev, Xin Wu, Fabrizio Tavecchio, I. Donnarumma, M. I. Martínez, Marco Tavani, J. Peyré, Elisa Bernardini, A. Argan, Roland Walter, J. Kiener, Piotr Orleanski, Mark Pearce, Ignasi Reichardt, A. Morselli, Andrzej A. Zdziarski, Martino Marisaldi, Vincent Tatischeff, Andrea Bulgarelli, Marica Branchesi, Uwe Oberlack, Rui Curado da Silva, Dieter H. Hartmann, Lorraine Hanlon, Philippe Laurent, Marco Ajello, D. Bernard, Valentina Fioretti, Martin Pohl, Alessio Aboudan, Gottfried Kanbach, Alessandro De Angelis, Gabriele Ghisellini, Stefan Funk, Peter von Ballmoos, Michele Doro, M. N. Mazziotta, Marco Roncadelli, Harald Ramarijaona, Roland Diehl, Margarita Hernanz, Alexei Ulyanov, G. Minervini, G. Piano, Riccardo Campana, Carl Budtz-Jørgensen, D. J. Thompson, M. Cardillo, Paolo De Coppi, Karl Mannheim, Roberto Turolla, Jürgen Knödlseder, Isabelle Grenier, A. Brogna
e-ASTROGAM (`enhanced ASTROGAM') is a breakthrough Observatory mission dedicated to the study of the non-thermal Universe in the photon energy range from 0.3 MeV to 3 GeV. The mission is based on an advanced space-proven detector technology, with unp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::489a4383388397451e1b6d1803076c9c
http://hdl.handle.net/11368/2921594
http://hdl.handle.net/11368/2921594
Autor:
Nicolas M. Barrière, José Alvarez, Andrei M. Bykov, Jürgen Knödlseder, Lorraine Hanlon, Pierre Jean, Rui Curado da Silva, Juan Manuel Del Cura Velayos, Peter von Ballmoos, Emmanuel Hinglais, Mark D. Leising, Jean Pierre Prost, Lucien Kuiper, Margarita Hernanz, John A. Tomsick, Tadayuki Takahashi, Filippo Frontera, Roland Walter, S. E. Boggs, Benoît Pirard, Jordi Isern, Andreas Zoglauer
Publikováno v:
SPIE Proceedings.
DUAL will study the origin and evolution of the elements and explores new frontiers of physics: extreme energies that drive powerful stellar explosions and accelerate particles to macroscopic energies; extreme densities that modify the laws of physic
Autor:
Julie McEnery, Alexander van der Horst, Alberto Dominguez, Alexander Moiseev, Alexandre Marcowith, Alice Harding, Amy Lien, Andrea Giuliani, Andrew Inglis, Stefano Ansoldi, Antonio Stamerra, Antonios Manousakis, Andy Strong, Cosimo Bambi, Barbara Patricelli, Matthew Baring, Juan Abel Barrio, Denis Bastieri, Brian Fields, John Beacom, Volker Beckmann, Wlodek Bednarek, Bindu Rani, Steven Boggs, Aleksey Bolotnikov, Brad Cenko, S., Jim Buckley, Brian Grefenstette, Michelle Hui, Carlotta Pittori, Chanda Prescod-Weinstein, Chris Shrader, Christian Gouiffes, Carolyn Kierans, Colleen Wilson-Hodge, Ammando, Filippo D., Daniel Castro, Daniel Kocveski, Dario Gasparrini, David Thompson, David Williams, Alessandro De Angelis, Denis Bernard, Seth Digel, Daniel Morcuende, Eric Charles, Elisabetta Bissaldi, Elizabeth Hays, Elizabeth Ferrara, Enrico Bozzo, Eric Grove, Eric Wulf, Eugenio Bottacini, Ezio Caroli, Fabian Kislat, Foteini Oikonomou, Francesco Giordano, Francesco Longo, Chris Fryer, Yasushi Fukazawa, Markos Georganopoulos, Georgia De Nolfo, Giacomo Vianello, Gottfried Kanbach, George Younes, Harsha Blumer, Dieter Hartmann, Margarita Hernanz, Hiromitsu Takahashi, Hui Li, Ivan Agudo, Igor Moskalenko, Inga Stumke, Isabelle Grenier, Jacob Smith, James Rodi, Jeremy Perkins, Joseph Gelfand, Jamie Holder, Jurgen Knodlseder, Joachim Kopp, Jean-Philippe Lenain, José-Manuel Álvarez, Jessica Metcalfe, John Krizmanic, Stephen, John B., Jack Hewitt, John Mitchell, Pat Harding, John Tomsick, Judith Racusin, Justin Finke, Oleg Kargaltsev, Klimenko, Alexei V., Henric Krawczynski, Karl Smith, Hidetoshi Kubo, Leonardo Di Venere, Lea Marcotulli, Jan Lommler, Lucas Parker, Luca Baldini, Luca Foffano, Luca Zampieri, Luigi Tibaldo, Maria Petropoulou, Marco Ajello, Manuel Meyer, Marcos López, Marc McConnell, Markus Boettcher, Martina Cardillo, Manel Martinez, Matthew Kerr, Nicola Mazziotta, M., Mattia Di Mauro, Matthew Wood, Eileen Meyer, Michael Briggs, Michaël De Becker, Michael Lovellette, Michele Doro, Sanchez-Conde, Miguel A., Michael Moss, Tsunefumi Mizuno, Marc Ribó, Kazuhiro Nakazawa, Naoko Kurahashi Neilson, Natalia Auricchio, Nicola Omodei, Uwe Oberlack, Masanori Ohno, Elena Orlando, Nepomuk Otte, Paolo Coppi, Peter Bloser, Haocheng Zhang, Philippe Laurent, Martin Pohl, Elisa Prandini, Peter Shawhan, Regina Caputo, Riccardo Campana, Riccardo Rando, Richard Woolf, Robert Johnson, Roberto Mignani, Roland Walter, Roopesh Ojha, Rui Curado da Silva, Stefano Dietrich, Stefan Funk, Silvia Zane, Sonia Anton, Sara Buson, Sara Cutini, Pablo Saz Parkinson, Richard Schirato, Sean Griffin, Kaufmann, S., Lukasz Stawarz, Stefano Ciprini, Stefano Del Sordo, Sam Jones, Sylvain Guiriec, Hiro Tajima, Teddy Cheung, Lih-Sin The, Tonia Venters, Troy Porter, Tim Linden, Ulisses Barres, Paliya, Vaidehi S., Vladimir Bozhilov, Tom Vestrand, Vincent Tatischeff, Wenlei Chen, Xilu Wang, Yasuyuki Tanaka, Lucas Uhm, Bing Zhang, Stephan Zimmer, Andreas Zoglauer, Zorawar Wadiasingh
Publikováno v:
INSPIRE-HEP
New York University Scholars
New York University Scholars
The All-sky Medium Energy Gamma-ray Observatory (AMEGO) is a probe class mission concept that will provide essential contributions to multimessenger astrophysics in the late 2020s and beyond. AMEGO combines high sensitivity in the 200 keV to 10 GeV e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5ce3ba9745fc7abe8932c4d9e6e5c787
http://inspirehep.net/record/1744303
http://inspirehep.net/record/1744303